Crystalline structure of the mixed confined-deconfined phase in neutron stars

Details Crystalline structure of the mixed confined-deconfined phase in neutron stars Crystalline structure of the mixed confined-deconfined phase in neutron stars

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995phrvc..52.2250g&link_type=abstract

Physical Review C (Nuclear Physics), Volume 52, Issue 4, October 1995, pp.2250-2253

Physics

Nuclear Physics

41

Neutron Stars, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Pulsars

Scientific paper

We calculate that the geometrical structure of the crystalline solid mixed phase of confined-deconfined hadronic matter in neutron stars-its form, size, spacing, and location in the star-is highly individualistic according to small changes in the stellar mass. This suggests a possible connection with the wide range of glitch behavior observed in different pulsars, since glitches are almost certainly associated with solid regions.

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